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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ACP</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7324</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-7-4149-2007</article-id>
<title-group>
<article-title>3-D polarised simulations of space-borne passive mm/sub-mm midlatitude cirrus observations: a case study</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Davis</surname>
<given-names>C. P.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Evans</surname>
<given-names>K. F.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Buehler</surname>
<given-names>S. A.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wu</surname>
<given-names>D. L.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Pumphrey</surname>
<given-names>H. C.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Institute of Atmospheric and Environmental Science, University of Edinburgh, Edinburgh, UK</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Dept. of Atmosphere and Oceanic Sciences, University of Colorado, Boulder, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Department of Space Science, Lulea Technical University, Kiruna, Sweden</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Jet Propulsion Laboratory, California Institute of Technology, Pasadena, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>07</day>
<month>08</month>
<year>2007</year>
</pub-date>
<volume>7</volume>
<issue>15</issue>
<fpage>4149</fpage>
<lpage>4158</lpage>
<permissions>
<license xlink:type="simple">
<license-p>This is an open-access article ditributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.</license-p>
</license>
</permissions>
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<self-uri xlink:href="http://www.atmos-chem-phys.net/7/4149/2007/acp-7-4149-2007.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/7/4149/2007/acp-7-4149-2007.pdf</self-uri>
<abstract>
<p>Global observations of ice clouds
are needed to improve our understanding of their
impact on earth&apos;s radiation balance and the water-cycle.
Passive mm/sub-mm has some advantages compared to other space-borne
cloud-ice remote sensing techniques.  The physics of scattering makes
forward radiative transfer modelling for such instruments challenging.
This paper demonstrates the ability of a recently developed RT code,
ARTS-MC, to accurately simulate
observations of this type for a variety of
viewing geometries corresponding to operational (AMSU-B, EOS-MLS) and
proposed (CIWSIR) instruments.
ARTS-MC employs an adjoint Monte-Carlo method, makes
proper account of polarisation, and uses 3-D spherical geometry.  The
actual field of view characteristics for each instrument are also
accounted for.  A 3-D midlatitude cirrus scenario is used, which
is derived from Chilbolton cloud radar data and a stochastic method
for generating 3-D ice water content fields.
These demonstration simulations clearly demonstrate the
beamfilling effect, significant polarisation effects for
non-spherical particles, and also a beamfilling effect with regard to
polarisation.</p>
</abstract>
<counts><page-count count="10"/></counts>
</article-meta>
</front>
<body/>
<back>
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</article>